Our analysis, combining weak lensing and clustering measurement,
clearly show that, at given \(M_*\) , the host halos of
quiescent galaxies are more massive than those of
star-forming galaxies and AGN host galaxies.
The difference is particularly significant in the two middle
\(M_*\)  bins, which include most (about 88%) of the AGNs.
It is in agreement with previous studies that found
quiescent galaxies reside in more massive halos than star-forming galaxies
of the same \(M_*\)[1]}, [2]}.
It is broadly consistent with the passive quenching model[3]},
in which star-forming galaxies grow faster than quiescent galaxies,
while their host halos grow in a statistically similar manner.
The host halo masses of AGN host are in good agreement
with those for star-forming galaxies, indicating that the
two populations of galaxies may be connected, as we will
discuss in Section .
